# Static spherically symmetric black holes in de Rham-Gabadadze-Tolley massive gravity in arbitrary dimensions

## TL;DR

This paper investigates static spherically symmetric black hole solutions in dRGT massive gravity across multiple dimensions, revealing two classes of solutions and an expression for the effective cosmological constant.

## Contribution

It provides new solutions in arbitrary dimensions and shows how the massive potential influences the effective cosmological constant in dRGT gravity.

## Key findings

- Two classes of black hole solutions identified
- Effective cosmological constant derived for arbitrary dimensions
- Massive potential impacts the cosmological constant effectively

## Abstract

This article is devoted to static spherically symmetric black hole solutions of dRGT (de Rham-Gabadadze-Tolley) massive gravity in the presence of cosmological constant. The unitary and non-unitary gauges are used to find the solutions in three, four and five dimensions. We show that there are two general classes of solutions. In one of them, the effect of massive potential is appeared as the effective cosmological constant. By investigating these solutions in different dimensions, we find an expression for effective cosmological constant in arbitrary dimensions.